氨水与金属离子对ADN基绿色推进剂稳定性影响

氨是ADN基绿色推进剂中常用的助剂,同时推进剂在储存与使用过程中,可能有微量过渡金属离子引入。为研究氨与金属离子对ADN基推进剂冰点与常温贮存稳定性的影响,本文采用GB/T 2430-2008的喷气燃料冰点测量法研究了氨对ADN-水体系冰点的影响,并采用美军标STANAG 4582的微量热加速老化法研究了氨与过渡金属离子对ADN-水体系常温贮存稳定性的影响。实验结果表明,氨在ADN推进剂体系中是一种优秀的助剂,可有效提升ADN基绿色推进剂的稳定性与使用温度范围。痕量Fe3+与Cr3+（≤15ppm）的引入使ADN基绿色推进剂的稳定性有小幅提升,而30ppm Fe3+、Cr3+与痕量Cu2+的引入使ADN推进剂稳定性略有下降,但仍在安全贮存使用标准范围内。可进一步探究氨与痕量Fe3+、Cr3+的最优化用量,以进一步优化ADN基绿色推进剂的组成,令其在使用性能与稳定性能间取得较好的平衡。     

材料非线性性质的解析表达

将材料拉伸实验曲线由比例极限到屈服极限（或名义屈服限）的非线性段，用一个含有四个参数的解析式子来表达。在此基础上，根据材料特性及最小二乘法原理，对９种金属材料的拉伸实验数据进行曲线拟合，得到各自相应的参数值。最后通过误差分析，验证了上述解析式的可用性，并阐述了它的实际意义。     

Laser Hardening of Metals

The first experiments on hardening metals by laserpeening induced residual compressive stress in the sur-face of metals for improving their resistance to cracking,stress corrosion and fatigue took place more than 30years ago. However, only today, with the development ofhigh-intensity pulse repetitive rate lasers, this methodstarts to compete to traditional peening, which use influ-ence of small metal balls.Laser peening uses pulses with high intensity 109￣1010 W/cm2 [1]. The laser energy abso…     

金属内衬纤维增强复合材料筒体设计

研究了金属内衬纤维增强复合材料筒体的设计方法,推导出了环向及螺旋加环向纤维缠绕的金属内衬筒体计算公式。以算例表明,该方法在保证壳体爆破强度前提下,达到了壳体减重和增加刚度的效果。本研究以固体火箭发动机壳体设计为背景,可以延伸用于一般压力容器。     

基于C/S的飞机钣金成形数据库系统的研究与开发

根据航空工业飞机生产、型号预研、钣金工艺手册、工艺试验等大量数据信息,以Oracle作为后台的数据库管理系统,采用PowerBuilder8.0作为前台的开发工具,研究开发了一套基于C／S,集中了板材性能、成形工艺、机床设备、工装、模具等数据资料的飞机钣金成形数据库系统。     

金属热防护系统的研究进展

简述国外几代金属热防护系统的发展概况，并论述金属热防护结构的组成特点，对金属热防护系统与其他传统热防护系统的优缺点进行比较，指出金属热防护系统必将是各种类型可重复使用航天飞行器大面积防热的最佳选择。     

金属橡胶挤压油膜阻尼器阻尼性能分析

为了降低发动机转子高速旋转产生的振动，提高发动机的使用寿命，设计了一种端部安装金属橡胶环的新型挤压油膜阻尼器，并在π油膜假设条件下，利用斯托克斯方程和雷诺方程，给出了新型金属橡胶挤压油膜阻尼器的流量表达式以及非线性油膜力的近似表达式。通过传统短挤压油膜阻尼器和新型金属橡胶挤压油膜阻尼器的流量特性和油膜力特性的对比分析，表明新型金属橡胶挤压油膜阻尼器具有更好的阻尼性能和良好的节流特性。并通过试验证明了新型金属橡胶挤压油膜阻尼器具有更好的阻尼减振效果。     

High-Latitude Particle Precipitation and its Relationship to Magnetospheric Source Regions

Two central issues in magnetospheric research are understanding the mapping of the low-altitude ionosphere to the distant regions of the magnetsphere, and understanding the relationship between the small-scale features detected in the various regions of the ionosphere and the global properties of the magnetosphere. The high-latitude ionosphere, through its magnetic connection to the outer magnetosphere, provides an important view of magnetospheric boundaries and the physical processes occurring there. All physical manifestations of this magnetic connectivity (waves, particle precipitation, etc.), however, have non-zero propagation times during which they are convected by the large-scale magnetospheric electric field, with phenomena undergoing different convection distances depending on their propagation times. Identification of the ionospheric signatures of magnetospheric regions and phenomena, therefore, can be difficult. Considerable progress has recently been made in identifying these convection signatures in data from low- and high-altitude satellites. This work has allowed us to learn much about issues such as: the rates of magnetic reconnection, both at the dayside magnetopause and in the magnetotail; particle transport across the open magnetopause; and particle acceleration at the magnetopause and the magnetotail current sheets.     

ISEE Ion Composition Data with Implications for Solar Wind Entry into Earth's Magnetotail

Energetic (0.1-16 keV/e) ion data from a plasma composition experiment on the ISEE-1 spacecraft show that Earth's plasma sheet (inside of 23 RE) always has a large population of H+ and He++ ions, the two principal ionic components of the solar wind. This population is the largest, in terms of both number density and spatial thickness, during extended periods of northward interplanetary magnetic field (IMF) and is then also the most "solar wind-like" in the sense that the He++/H+ density ratio is at its peak (about 3% on average in 1978 and 79) and the H+ and He++ have mean (thermal) energies that are in the ratio of about 1:4 and barely exceed the typical bulk flow energy in the solar wind. During geomagnetically active times, associated with southward turnings of the IMF, the H+ and He++ are heated in the central plasma sheet, and reduced in density. Even when the IMF is southward, these ions can be found with lower solar wind-like energies closer to the tail lobes, at least during plasma sheet thinning in the early phase of substorms, when they are often seen to flow tailward, approximately along the magnetic field, at a slow to moderate speed (of order 100 km s-1 or less). These tailward flows, combined with the large density and generally solar wind-like energies of plasma sheet H+ and He++ ions during times of northward IMF, are interpreted to mean that the solar wind enters along the tail flanks, in a region between the lobes and the central plasma sheet, propelled inward by ExB drift associated with the electric fringe field of the low latitude magnetopause boundary layer (LLBL). In order to complete this scenario, it is argued that the rapid (of order 1000 km s-1) earthward ion flows (mostly H+ ions), also along the magnetic field, that are more typically the precursors of plasma sheet "recovery" during substorm expansion, are not proof of solar wind entry in the distant tail, but may instead be a time-of-flight effect associated with plasma sheet redistribution in a dipolarizing magnetic field.     

高能量密度燃料HDF-1与金属材料的相容性

研究了高能量密度燃料HDF－1在贮存使用过程中与可能接触到的金属材料的相互影响，通过升温加速的实验方法，考察了燃料对金属表面的影响以及金属材料对燃料氧化的影响，结果表明，HDF－1对钛，铝金属表面无影响，对铜表面的影响小于3^#航空煤油（RP－3），铝，钛，铝镍合金对燃料体系无影响，而铜，铁对燃料氧化具有明显的催化作用，进一步研究表明，铁具有更强的作用效果，通过对照实验发现HDF－1与材料的相容性优于RP－3。